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TOI-5344 b: A Saturn-like planet orbiting a super-Solar metallicity M0 dwarf

We confirm the planetary nature of TOI-5344 b as a transiting giant exoplanet around an M0 dwarf star. TOI-5344 b was discovered with the Transiting Exoplanet Survey Satellite photometry and confirmed with ground-based photometry (the Red Buttes Observatory 0.6m telescope), radial velocity (the Habi...

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Published in:arXiv.org 2023-11
Main Authors: Han, Te, Robertson, Paul, Kanodia, Shubham, Cañas, Caleb, Lin, Andrea S J, Stefánsson, Guðmundur, Libby-Roberts, Jessica E, Larsen, Alexander, Kobulnicky, Henry A, Mahadevan, Suvrath, Bender, Chad F, Cochran, William D, Endl, Michael, Everett, Mark E, Gupta, Arvind F, Halverson, Samuel, Hearty, Fred, Monson, Andrew, Ninan, Joe P, Roy, Arpita, Schwab, Christian, Terrien, Ryan C
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container_title arXiv.org
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creator Han, Te
Robertson, Paul
Kanodia, Shubham
Cañas, Caleb
Lin, Andrea S J
Stefánsson, Guðmundur
Libby-Roberts, Jessica E
Larsen, Alexander
Kobulnicky, Henry A
Mahadevan, Suvrath
Bender, Chad F
Cochran, William D
Endl, Michael
Everett, Mark E
Gupta, Arvind F
Halverson, Samuel
Hearty, Fred
Monson, Andrew
Ninan, Joe P
Roy, Arpita
Schwab, Christian
Terrien, Ryan C
description We confirm the planetary nature of TOI-5344 b as a transiting giant exoplanet around an M0 dwarf star. TOI-5344 b was discovered with the Transiting Exoplanet Survey Satellite photometry and confirmed with ground-based photometry (the Red Buttes Observatory 0.6m telescope), radial velocity (the Habitable-zone Planet Finder), and speckle imaging (the NN-Explore Exoplanet Stellar Speckle Imager). TOI-5344 b is a Saturn-like giant planet (\(\rho = 0.80^{+0.17}_{-0.15}\ \text{g cm}^{-3}\)) with a planetary radius of \(9.7 \pm \ 0.5 \ \text{R}_{\oplus}\) (\(0.87 \pm \ 0.04 \ \text{R}_{\text{Jup}}\)) and a planetary mass of \(135^{+17}_{-18} \text{M}_{\oplus}\) (\(0.42^{+0.05}_{-0.06} \ \text{M}_{\text{Jup}}\)). It has an orbital period of \(3.792622 \pm 0.000010\) days and an orbital eccentricity of \(0.06^{+0.07}_{-0.04}\). We measure a high metallicity for TOI-5344 of [Fe/H] = \(0.48 \pm 0.12\), where the high metallicity is consistent with expectations from formation through core accretion. We compare the metallicity of the M-dwarf hosts of giant exoplanets to that of M-dwarf hosts of non-giants (\(\lesssim 8\ \text{R}_{\oplus}\)). While the two populations appear to show different metallicity distributions, quantitative tests are prohibited by various sample caveats.
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subjects Buttes
Circumstellar habitable zone
Deposition
Extrasolar planets
Metallicity
Orbits
Photometry
Planet detection
Planetary mass
Radial velocity
Red dwarf stars
Transit
title TOI-5344 b: A Saturn-like planet orbiting a super-Solar metallicity M0 dwarf
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